SuperDARN CUTLASS Finland radar observations of high-latitude magnetic reconnections under northward interplanetary magnetic field (IMF) conditions
Abstract A number of backscatter power enhancement events with “equatorward-moving radar auroral forms” in the high-latitude ionosphere were observed by SuperDARN CUTLASS Finland radar when the IMF was northward during 09:00–10:00 UT on 26 March 2004. These events were also associated with sunward f...
Ausführliche Beschreibung
Autor*in: |
Zhang, QingHe [verfasserIn] Liu, RuiYuan [verfasserIn] Yang, HuiGen [verfasserIn] Hu, HongQiao [verfasserIn] Zhang, BeiChen [verfasserIn] Dunlop, Malcolm [verfasserIn] Lester, Mark [verfasserIn] Bogdanova, Yulia [verfasserIn] Walsh, Andrew [verfasserIn] |
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E-Artikel |
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Sprache: |
Englisch |
Erschienen: |
2012 |
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Schlagwörter: |
high-latitude magnetic reconnection |
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Übergeordnetes Werk: |
Enthalten in: Science in China - Heidelberg : Springer, 1997, 55(2012), 5 vom: 21. März, Seite 1207-1216 |
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Übergeordnetes Werk: |
volume:55 ; year:2012 ; number:5 ; day:21 ; month:03 ; pages:1207-1216 |
Links: |
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DOI / URN: |
10.1007/s11431-012-4820-y |
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Katalog-ID: |
SPR019275625 |
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520 | |a Abstract A number of backscatter power enhancement events with “equatorward-moving radar auroral forms” in the high-latitude ionosphere were observed by SuperDARN CUTLASS Finland radar when the IMF was northward during 09:00–10:00 UT on 26 March 2004. These events were also associated with sunward flow enhancements at each location in the Northern Hemisphere which were shown in ionospheric convections measured by the SuperDARN radars. These are typical features of high-latitude (lobe) magnetic reconnections. The durations of the velocity enhancements imply that the evolution time of the lobe reconnections is about 8–16 min from their origin at the reconnection site to their addition to the magnetotail lobe again. In additional, the Double Star TC-1 spacecraft was moving from magnetosheath into magnetosphere, and crossing the magnetopause near the subsolar region during this interval, and observed typical low-latitude magnetic reconnection signatures. This infers that the dayside high- and low-latitude reconnections may occur simultaneously. | ||
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650 | 4 | |a evolution time of the lobe reconnections |7 (dpeaa)DE-He213 | |
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700 | 1 | |a Zhang, BeiChen |e verfasserin |4 aut | |
700 | 1 | |a Dunlop, Malcolm |e verfasserin |4 aut | |
700 | 1 | |a Lester, Mark |e verfasserin |4 aut | |
700 | 1 | |a Bogdanova, Yulia |e verfasserin |4 aut | |
700 | 1 | |a Walsh, Andrew |e verfasserin |4 aut | |
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10.1007/s11431-012-4820-y doi (DE-627)SPR019275625 (SPR)s11431-012-4820-y-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Zhang, QingHe verfasserin aut SuperDARN CUTLASS Finland radar observations of high-latitude magnetic reconnections under northward interplanetary magnetic field (IMF) conditions 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract A number of backscatter power enhancement events with “equatorward-moving radar auroral forms” in the high-latitude ionosphere were observed by SuperDARN CUTLASS Finland radar when the IMF was northward during 09:00–10:00 UT on 26 March 2004. These events were also associated with sunward flow enhancements at each location in the Northern Hemisphere which were shown in ionospheric convections measured by the SuperDARN radars. These are typical features of high-latitude (lobe) magnetic reconnections. The durations of the velocity enhancements imply that the evolution time of the lobe reconnections is about 8–16 min from their origin at the reconnection site to their addition to the magnetotail lobe again. In additional, the Double Star TC-1 spacecraft was moving from magnetosheath into magnetosphere, and crossing the magnetopause near the subsolar region during this interval, and observed typical low-latitude magnetic reconnection signatures. This infers that the dayside high- and low-latitude reconnections may occur simultaneously. high-latitude magnetic reconnection (dpeaa)DE-He213 equatorward-moving radar auroral form (dpeaa)DE-He213 evolution time of the lobe reconnections (dpeaa)DE-He213 Liu, RuiYuan verfasserin aut Yang, HuiGen verfasserin aut Hu, HongQiao verfasserin aut Zhang, BeiChen verfasserin aut Dunlop, Malcolm verfasserin aut Lester, Mark verfasserin aut Bogdanova, Yulia verfasserin aut Walsh, Andrew verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 55(2012), 5 vom: 21. März, Seite 1207-1216 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:55 year:2012 number:5 day:21 month:03 pages:1207-1216 https://dx.doi.org/10.1007/s11431-012-4820-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 55 2012 5 21 03 1207-1216 |
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10.1007/s11431-012-4820-y doi (DE-627)SPR019275625 (SPR)s11431-012-4820-y-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Zhang, QingHe verfasserin aut SuperDARN CUTLASS Finland radar observations of high-latitude magnetic reconnections under northward interplanetary magnetic field (IMF) conditions 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract A number of backscatter power enhancement events with “equatorward-moving radar auroral forms” in the high-latitude ionosphere were observed by SuperDARN CUTLASS Finland radar when the IMF was northward during 09:00–10:00 UT on 26 March 2004. These events were also associated with sunward flow enhancements at each location in the Northern Hemisphere which were shown in ionospheric convections measured by the SuperDARN radars. These are typical features of high-latitude (lobe) magnetic reconnections. The durations of the velocity enhancements imply that the evolution time of the lobe reconnections is about 8–16 min from their origin at the reconnection site to their addition to the magnetotail lobe again. In additional, the Double Star TC-1 spacecraft was moving from magnetosheath into magnetosphere, and crossing the magnetopause near the subsolar region during this interval, and observed typical low-latitude magnetic reconnection signatures. This infers that the dayside high- and low-latitude reconnections may occur simultaneously. high-latitude magnetic reconnection (dpeaa)DE-He213 equatorward-moving radar auroral form (dpeaa)DE-He213 evolution time of the lobe reconnections (dpeaa)DE-He213 Liu, RuiYuan verfasserin aut Yang, HuiGen verfasserin aut Hu, HongQiao verfasserin aut Zhang, BeiChen verfasserin aut Dunlop, Malcolm verfasserin aut Lester, Mark verfasserin aut Bogdanova, Yulia verfasserin aut Walsh, Andrew verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 55(2012), 5 vom: 21. März, Seite 1207-1216 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:55 year:2012 number:5 day:21 month:03 pages:1207-1216 https://dx.doi.org/10.1007/s11431-012-4820-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 55 2012 5 21 03 1207-1216 |
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10.1007/s11431-012-4820-y doi (DE-627)SPR019275625 (SPR)s11431-012-4820-y-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Zhang, QingHe verfasserin aut SuperDARN CUTLASS Finland radar observations of high-latitude magnetic reconnections under northward interplanetary magnetic field (IMF) conditions 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract A number of backscatter power enhancement events with “equatorward-moving radar auroral forms” in the high-latitude ionosphere were observed by SuperDARN CUTLASS Finland radar when the IMF was northward during 09:00–10:00 UT on 26 March 2004. These events were also associated with sunward flow enhancements at each location in the Northern Hemisphere which were shown in ionospheric convections measured by the SuperDARN radars. These are typical features of high-latitude (lobe) magnetic reconnections. The durations of the velocity enhancements imply that the evolution time of the lobe reconnections is about 8–16 min from their origin at the reconnection site to their addition to the magnetotail lobe again. In additional, the Double Star TC-1 spacecraft was moving from magnetosheath into magnetosphere, and crossing the magnetopause near the subsolar region during this interval, and observed typical low-latitude magnetic reconnection signatures. This infers that the dayside high- and low-latitude reconnections may occur simultaneously. high-latitude magnetic reconnection (dpeaa)DE-He213 equatorward-moving radar auroral form (dpeaa)DE-He213 evolution time of the lobe reconnections (dpeaa)DE-He213 Liu, RuiYuan verfasserin aut Yang, HuiGen verfasserin aut Hu, HongQiao verfasserin aut Zhang, BeiChen verfasserin aut Dunlop, Malcolm verfasserin aut Lester, Mark verfasserin aut Bogdanova, Yulia verfasserin aut Walsh, Andrew verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 55(2012), 5 vom: 21. März, Seite 1207-1216 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:55 year:2012 number:5 day:21 month:03 pages:1207-1216 https://dx.doi.org/10.1007/s11431-012-4820-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 55 2012 5 21 03 1207-1216 |
allfieldsGer |
10.1007/s11431-012-4820-y doi (DE-627)SPR019275625 (SPR)s11431-012-4820-y-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Zhang, QingHe verfasserin aut SuperDARN CUTLASS Finland radar observations of high-latitude magnetic reconnections under northward interplanetary magnetic field (IMF) conditions 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract A number of backscatter power enhancement events with “equatorward-moving radar auroral forms” in the high-latitude ionosphere were observed by SuperDARN CUTLASS Finland radar when the IMF was northward during 09:00–10:00 UT on 26 March 2004. These events were also associated with sunward flow enhancements at each location in the Northern Hemisphere which were shown in ionospheric convections measured by the SuperDARN radars. These are typical features of high-latitude (lobe) magnetic reconnections. The durations of the velocity enhancements imply that the evolution time of the lobe reconnections is about 8–16 min from their origin at the reconnection site to their addition to the magnetotail lobe again. In additional, the Double Star TC-1 spacecraft was moving from magnetosheath into magnetosphere, and crossing the magnetopause near the subsolar region during this interval, and observed typical low-latitude magnetic reconnection signatures. This infers that the dayside high- and low-latitude reconnections may occur simultaneously. high-latitude magnetic reconnection (dpeaa)DE-He213 equatorward-moving radar auroral form (dpeaa)DE-He213 evolution time of the lobe reconnections (dpeaa)DE-He213 Liu, RuiYuan verfasserin aut Yang, HuiGen verfasserin aut Hu, HongQiao verfasserin aut Zhang, BeiChen verfasserin aut Dunlop, Malcolm verfasserin aut Lester, Mark verfasserin aut Bogdanova, Yulia verfasserin aut Walsh, Andrew verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 55(2012), 5 vom: 21. März, Seite 1207-1216 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:55 year:2012 number:5 day:21 month:03 pages:1207-1216 https://dx.doi.org/10.1007/s11431-012-4820-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 55 2012 5 21 03 1207-1216 |
allfieldsSound |
10.1007/s11431-012-4820-y doi (DE-627)SPR019275625 (SPR)s11431-012-4820-y-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Zhang, QingHe verfasserin aut SuperDARN CUTLASS Finland radar observations of high-latitude magnetic reconnections under northward interplanetary magnetic field (IMF) conditions 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract A number of backscatter power enhancement events with “equatorward-moving radar auroral forms” in the high-latitude ionosphere were observed by SuperDARN CUTLASS Finland radar when the IMF was northward during 09:00–10:00 UT on 26 March 2004. These events were also associated with sunward flow enhancements at each location in the Northern Hemisphere which were shown in ionospheric convections measured by the SuperDARN radars. These are typical features of high-latitude (lobe) magnetic reconnections. The durations of the velocity enhancements imply that the evolution time of the lobe reconnections is about 8–16 min from their origin at the reconnection site to their addition to the magnetotail lobe again. In additional, the Double Star TC-1 spacecraft was moving from magnetosheath into magnetosphere, and crossing the magnetopause near the subsolar region during this interval, and observed typical low-latitude magnetic reconnection signatures. This infers that the dayside high- and low-latitude reconnections may occur simultaneously. high-latitude magnetic reconnection (dpeaa)DE-He213 equatorward-moving radar auroral form (dpeaa)DE-He213 evolution time of the lobe reconnections (dpeaa)DE-He213 Liu, RuiYuan verfasserin aut Yang, HuiGen verfasserin aut Hu, HongQiao verfasserin aut Zhang, BeiChen verfasserin aut Dunlop, Malcolm verfasserin aut Lester, Mark verfasserin aut Bogdanova, Yulia verfasserin aut Walsh, Andrew verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 55(2012), 5 vom: 21. März, Seite 1207-1216 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:55 year:2012 number:5 day:21 month:03 pages:1207-1216 https://dx.doi.org/10.1007/s11431-012-4820-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 55 2012 5 21 03 1207-1216 |
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These events were also associated with sunward flow enhancements at each location in the Northern Hemisphere which were shown in ionospheric convections measured by the SuperDARN radars. These are typical features of high-latitude (lobe) magnetic reconnections. The durations of the velocity enhancements imply that the evolution time of the lobe reconnections is about 8–16 min from their origin at the reconnection site to their addition to the magnetotail lobe again. In additional, the Double Star TC-1 spacecraft was moving from magnetosheath into magnetosphere, and crossing the magnetopause near the subsolar region during this interval, and observed typical low-latitude magnetic reconnection signatures. 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Zhang, QingHe |
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600 ASE 50.00 bkl SuperDARN CUTLASS Finland radar observations of high-latitude magnetic reconnections under northward interplanetary magnetic field (IMF) conditions high-latitude magnetic reconnection (dpeaa)DE-He213 equatorward-moving radar auroral form (dpeaa)DE-He213 evolution time of the lobe reconnections (dpeaa)DE-He213 |
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SuperDARN CUTLASS Finland radar observations of high-latitude magnetic reconnections under northward interplanetary magnetic field (IMF) conditions |
abstract |
Abstract A number of backscatter power enhancement events with “equatorward-moving radar auroral forms” in the high-latitude ionosphere were observed by SuperDARN CUTLASS Finland radar when the IMF was northward during 09:00–10:00 UT on 26 March 2004. These events were also associated with sunward flow enhancements at each location in the Northern Hemisphere which were shown in ionospheric convections measured by the SuperDARN radars. These are typical features of high-latitude (lobe) magnetic reconnections. The durations of the velocity enhancements imply that the evolution time of the lobe reconnections is about 8–16 min from their origin at the reconnection site to their addition to the magnetotail lobe again. In additional, the Double Star TC-1 spacecraft was moving from magnetosheath into magnetosphere, and crossing the magnetopause near the subsolar region during this interval, and observed typical low-latitude magnetic reconnection signatures. This infers that the dayside high- and low-latitude reconnections may occur simultaneously. |
abstractGer |
Abstract A number of backscatter power enhancement events with “equatorward-moving radar auroral forms” in the high-latitude ionosphere were observed by SuperDARN CUTLASS Finland radar when the IMF was northward during 09:00–10:00 UT on 26 March 2004. These events were also associated with sunward flow enhancements at each location in the Northern Hemisphere which were shown in ionospheric convections measured by the SuperDARN radars. These are typical features of high-latitude (lobe) magnetic reconnections. The durations of the velocity enhancements imply that the evolution time of the lobe reconnections is about 8–16 min from their origin at the reconnection site to their addition to the magnetotail lobe again. In additional, the Double Star TC-1 spacecraft was moving from magnetosheath into magnetosphere, and crossing the magnetopause near the subsolar region during this interval, and observed typical low-latitude magnetic reconnection signatures. This infers that the dayside high- and low-latitude reconnections may occur simultaneously. |
abstract_unstemmed |
Abstract A number of backscatter power enhancement events with “equatorward-moving radar auroral forms” in the high-latitude ionosphere were observed by SuperDARN CUTLASS Finland radar when the IMF was northward during 09:00–10:00 UT on 26 March 2004. These events were also associated with sunward flow enhancements at each location in the Northern Hemisphere which were shown in ionospheric convections measured by the SuperDARN radars. These are typical features of high-latitude (lobe) magnetic reconnections. The durations of the velocity enhancements imply that the evolution time of the lobe reconnections is about 8–16 min from their origin at the reconnection site to their addition to the magnetotail lobe again. In additional, the Double Star TC-1 spacecraft was moving from magnetosheath into magnetosphere, and crossing the magnetopause near the subsolar region during this interval, and observed typical low-latitude magnetic reconnection signatures. This infers that the dayside high- and low-latitude reconnections may occur simultaneously. |
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title_short |
SuperDARN CUTLASS Finland radar observations of high-latitude magnetic reconnections under northward interplanetary magnetic field (IMF) conditions |
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These events were also associated with sunward flow enhancements at each location in the Northern Hemisphere which were shown in ionospheric convections measured by the SuperDARN radars. These are typical features of high-latitude (lobe) magnetic reconnections. The durations of the velocity enhancements imply that the evolution time of the lobe reconnections is about 8–16 min from their origin at the reconnection site to their addition to the magnetotail lobe again. In additional, the Double Star TC-1 spacecraft was moving from magnetosheath into magnetosphere, and crossing the magnetopause near the subsolar region during this interval, and observed typical low-latitude magnetic reconnection signatures. 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